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Radiation Pressure Calculator (light pressure, force and solar-sail acceleration)

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Understanding the radiation pressure calculator — concept and principle

This calculator finds the pressure light exerts on a surface from its intensity and the surface's reflectance, and the resulting force, acceleration and speed gained per day for a given area and mass. It is used for solar-sail examples, spacecraft orbit perturbations and physics courses.

Radiation pressure on a sailSunlight pushing a solar sailIntensity1,370 W/m²Reflectivity · area100 % · 32 m²Mass5 kgp = 2 × 1,370 ÷ c = 9.14 µPaF = 9.14 µPa × 32 m²Force0.0002925 NAcceleration0.00005849 m/s²Speed gained per day5.054 m/s
Light carries momentum; a mirror reverses it, doubling the push. Tiny, but it never stops.

How it is calculated

p = (1 + R) × I ÷ c

Absorber: p = I ÷ c; perfect mirror: p = 2I ÷ c

Force F = p × A; acceleration a = F ÷ m; speed per day = a × 86,400 s

The principle

Light carries momentum as well as energy: a beam of power P carries momentum P/c per second. When it is absorbed, that momentum is transferred to the surface; when it is reflected, the light's momentum reverses, so the surface receives twice as much. The pressure is tiny because c is so large, but in space there is no friction, so even a tiny steady push builds up speed over days and months.

Worked example

Default inputs: I = 1,370 W/m² (sunlight near Earth), R = 100%, A = 32 m², m = 5 kg.

  1. p = 2 × 1,370 ÷ 299,792,458 = 9.14 µPa (0.00000914 Pa).
  2. F = 9.14 × 10⁻⁶ × 32 = 0.0002925 N.
  3. a = 0.0002925 ÷ 5 = 0.00005849 m/s².
  4. Speed gained per day = 0.00005849 × 86,400 = 5.054 m/s.
  5. A perfect absorber would feel half: 4.57 µPa.

How to read the result

Sunlight at Earth's distance pushes with only a few micropascals, about one ten-billionth of atmospheric pressure. Yet a light solar sail gains several metres per second each day, which over months is useful propulsion. The pressure falls with the square of distance from the Sun.

Common mistakes

Keep in mind: The model assumes light hitting the surface head-on and ignores gravity, thermal re-emission and sail shape.

Frequently asked questions

How strong is sunlight's pressure on Earth?

About 4.6 µPa on an absorber and 9.1 µPa on a mirror.

Why does reflection double the pressure?

The light's momentum is reversed, so twice the momentum is transferred.

Can radiation pressure move spacecraft?

Yes; solar-sail missions have demonstrated it.

Does it affect satellites?

Yes, it slightly perturbs orbits and must be included in precise tracking.

Sources: OpenStax, University Physics Volume 2 (2016), section 16.4 "Momentum and Radiation Pressure"

Checked 9 Nov 2026. OpenStax, University Physics Volume 2 (2016), section 16.4 “Momentum and Radiation Pressure”, Equation 16.36: p = I/c (absorber), p = 2I/c (perfect reflector); Example 16.7 (LightSail: 1,370 W/m², 32 m², 5.0 kg → F ≈ 2.92 × 10⁻⁴ N). Speed of light c exact (SI).

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